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Infrared excesses and mass loss: Implications for OB stars in Carina and the LMC

Published online by Cambridge University Press:  14 August 2015

A. R. Hyland
A. R. Hyland*
Affiliation:
Mount Stromlo and Siding Spring Observatories, The Australian National University, Canberra, Australia

Abstract

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A method of deriving mass loss rates using near IR excesses is established and applied to OB stars in Carina and the LMC.

Type
Session 3: Infrared and Radio Data
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 143 - 146
Copyright
Copyright © Reidel 1979 

References

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